Dense metal planets like Mercury are probably rare in the universe

September 6, 2018 by Matt Williams, Universe Today

The planet Mercury, the closet planet to our Sun, is something of an exercise in extremes. It's days last longer than it's years and at any given time, it's sun-facing side is scorching hot while its dark side is freezing cold. It is also one of the least understood planets in our solar system. While it is a terrestrial (i.e. rocky) planet like Earth, Venus and Mars, it has a significantly higher iron-to-rock ratio than the others.

For decades, the most widely-accepted theory for this was that Mercury experienced a massive in the past which caused the planet to shed much of its rocky mantle. However, according to a new study by a team of scientists from the Center for Theoretical Astrophysics and Cosmology (CTAC) at the University of Zurich, Mercury's mysterious nature may actually be the result of multiple collisions with giant objects.

For the sake of their study, titled "Forming Mercury by Giant Impacts," team leader Alice Chau and her colleagues (all of whom are members with the Institute for Computational Science at the CTAC) considered the various reasons for why Mercury has the density and iron-to-rock ratio that it does. In the end, they considered all the possible scenarios to determine which was the most likely one.

To break it down, Mercury has remained something of a mystery to astronomers because of its much more metallic than its neighbors. Much like Earth, Venus and Mars, Mercury is a terrestrial planet, meaning that it is composed of silicate minerals and metals that are differentiated into an iron core and silicate mantle and crust. But unlike the other rocky planets of the solar system, iron makes up a disproportionately large amount of the planet.

Internal structure of Mercury: 1. Crust: 100–300 km thick 2. Mantle: 600 km thick 3. Core: 1,800 km radius. Credit: NASA/JPL

Not only does Mercury's core have a higher iron content that any other major planet in the solar system, but based on its density and size, geologists estimate that Mercury's core occupies about 42 percent of its volume – compared to Earth's 17 percent. The reason for this remains unknown, but many theories have been advanced over the years. As Chau told universe Today via email, these theories can be divided into two categories:

Either Mercury acquired its large iron core from the beginning on, in the solar nebula/disk. Close to the Sun some mechanisms might have been more efficient to separate metals and rocks (because of their different condensation temperature, or conductive properties, or their balance between drag force and gravity), which would drift more metals inward and rocks outward. Mercury would then form at a location more metal-rich than in the rest of the disk. ii) or it formed a core similar in mass ratio than the other terrestrial planets but lost part of its mantle in the late stages of its formation, like in a giant impact or by evaporation (and the vapor mantle would be blown away by solar winds)."

The second possibility, where Mercury lost much of its mantle due to evaporation or a massive impact, remains the most widely-accepted among the scientific community. Building on this, Chau and her colleagues studied standard collision parameters (impact velocity, mass ratio, impact parameter) and considered what an impactor's likely composition would be, as well as how the cooling of Mercury afterwards would play a role.

Artist view of the MESSENGER spacecraft orbiting the innermost planet Mercury. Credit: NASA

The purpose of this was to determine if Mercury's composition was the result of a single, giant impact, or many smaller ones. While both possibilities are rare and would require a unique set of circumstances, Chau and her colleagues determined that either impact scenarios could account for Mercury's curious nature. As she explained, their conclusions came down to five points:

  1. A single giant impact or hit-and-run impact require a highly tuned impact parameter and velocity to reproduce Mercury's mass and iron mass fraction. There is a somewhat larger parameter space of possibilities in the hit-and-run scenario.
  2. The impactor's composition affects the resulting final mass and post-impact iron distribution.
  3. The pre-impact state of the target affects the resulting final mass.
  4. A multiple-collision scenario escapes the fine-tuning of the geometrical parameters but is constrained by the timing and by the volatile-rich composition of Mercury's surface.
  5. Forming Mercury by giant impacts is feasible but difficult.

In short, they found that it is possible that both scenarios could account for Mercury's high iron-to-rock ration, but that the odds of them having happened are not great. This is supported, according to Chau, by the fact that few Mercury-analog exoplanets have been found. In this respect, whatever caused Mercury to become the way it is may be a relatively rare event as far as the evolution of star systems are concerned.

Artist’s impression of the impact that caused the formation of the moon. Credit: NASA/GSFC
"Our study isn't the first one to propose giant impacts to explain Mercury's large , but confirms that we need rather specific conditions for giant impacts," said Chau. "It seems that forming Mercury is difficult. In another sense, this is reassuring because we do not observe a lot of exoplanets that are similar to Mercury in composition. Also, even if it is a rare event, only one impact is needed."

In this sense, giant impacts could be seen as fortunate events and a reminder of how chaotic planetary systems are, Chau added. For not only do these types of collisions have a profound impact on a planet's properties (for instance, the Earth-moon system is believed to be the result of a giant impact), but based on exoplanet surveys, such instances also appear to be quite rare.

Perhaps our solar system is unique in several respects, which include the emergence of life and the presence of giant impacts that fundamentally altered several of its planets. Then again, we have really only begun to scratch the surface as far as exoplanet discoveries are concerned, and we may find many Mercury-like out there yet.

Explore further: Newly-discovered planet is hot, metallic and dense as Mercury (Update)

More information: Forming Mercury by Giant Impacts:

Related Stories

Geologists identify the mineralogy of Mercury

December 21, 2016

For the first time, geologists from the University of Liège have been able to determine the nature of the minerals present on the surface of Mercury - one of the four telluric planets in our solar system. Their study, published ...

New estimates of Mercury's thin, dense crust

April 27, 2018

Mercury is small, fast and close to the sun, making the rocky world challenging to visit. Only one probe has ever orbited the planet and collected enough data to tell scientists about the chemistry and landscape of Mercury's ...

Earth's carbon points to planetary smashup

September 5, 2016

Research by Rice University Earth scientists suggests that virtually all of Earth's life-giving carbon could have come from a collision about 4.4 billion years ago between Earth and an embryonic planet similar to Mercury.

Recommended for you

Female golden snub-nosed monkeys share nursing of young

February 21, 2019

An international team of researchers including The University of Western Australia and China's Central South University of Forestry and Technology has discovered that female golden snub-nosed monkeys in China are happy to ...

When does one of the central ideas in economics work?

February 20, 2019

The concept of equilibrium is one of the most central ideas in economics. It is one of the core assumptions in the vast majority of economic models, including models used by policymakers on issues ranging from monetary policy ...

In colliding galaxies, a pipsqueak shines bright

February 20, 2019

In the nearby Whirlpool galaxy and its companion galaxy, M51b, two supermassive black holes heat up and devour surrounding material. These two monsters should be the most luminous X-ray sources in sight, but a new study using ...

Research reveals why the zebra got its stripes

February 20, 2019

Why do zebras have stripes? A study published in PLOS ONE today takes us another step closer to answering this puzzling question and to understanding how stripes actually work.


Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.